TCF-S Details

Unique to the TCF-S focuser, an electronic controller system monitors the telescope's tube temperature and compensates the focus accordingly.
A small temperature probe is attached to the side of the telescope tube and monitors temperature with a resolution of 0.1° C. For a typical
Schmidt-Cassegrain of 8 to 11 inches aperture and f/10 focal ratio, the back-focus will move approximately 0.010 inches for every 1° C change in
temperature. It is not unusual during an observing session for the ambient temperature to change by as much as 10° C within the time span of a few hours.
This change in focus due to temperature is a serious problem for most telescope designs and requires frequent re-focusing during long
exposures. A typical RGB exposure sequence can last one hour or more making it imperative that the focus be checked and corrected after each filter change.

A simple setup procedure is used to find the temperature coefficients specific to the user's telescope system. The TCF-S system allows for two
different coefficients (corresponding to two different f-ratio configurations) to be calculated and stored in the EEPROM memory. Once learned, either
coefficient can be selected with a simple slide switch. A manual mode allows the user to set the focus manually at any time.

The digital nature of the TCF-S allows opportunities for truly intelligent focusing. With the TCF-S focuser, programmers can communicate directly
with the focuser's controller (located in the hand control) via any serial port. The simple ASCII protocol is easily programmed and has been implemented
in many popular imaging and camera control software packages. For example, CCDSoft Version 5 offers the @Focus routine which communicates with the TCF-S
via a serial port to provide truly automatic focus control. MaxIm DL/CCD version 3 and above provides remote and automatic focus control with the TCF-S focuser.

At the end of an observing session, the TCF-S focuser remembers the last temperature and position. When the unit is turned back on for a new session,
the TCF-S computes a new position using the current tube temperature and moves to that position. Assuming no changes to the optical configuration, the
object will snap into sharp focus. It is possible to observe many days without the need to focus again.

The TCF-S comes with its own PC control program for Windows. The source code for the program is available in the TCF-S folder after the install program is run.
Users are encouraged to write their operating program using the TCF-S.bas routines as examples. You can download the setup program for TCF-S_Control by going to
our Software Download page. The navigation button is on the left.